Resonant ion-dip infrared spectroscopy of benzene(methanol)m clusters with m=16
J. Chem. Phys. 106, 2145 (1997); doi:10.1063/1.473784
Issue Date: 8 February 1997
You are not logged in to this journal. Log in
Resonant ion-dip infrared spectroscopy has been employed to record cluster-size-specific spectra of C6H6(CH3OH)m with m=16 in the OH stretch fundamental region. The comparison of the spectra with the results of ab initio calculations on the pure methanol clusters enables the assignment of the hydrogen-bonding architecture in the clusters. In all cases, the methanol molecules aggregate together in a single subcluster. With m=1, a single infrared transition is observed, redshifted from that of a free methanol momomer by 42 cm1 due to
hydrogen bonding between benzene and methanol. The m=2 spectrum features two strong transitions at 3506 and 3605 cm1. The lower frequency peak is redshifted from the free monomer value by 175 cm1 and is assigned to the proton donor in the methanol dimer subcluster. The proton acceptor, which would be a free OH stretch in the absence of benzene, is redshifted by 76 cm1 due to a strengthened
hydrogen bond. In benzene(CH3OH)3, three sharp OH stretch transitions are observed at 3389, 3435, and 3589 cm1. The comparison of these absorptions with ab initio calculations and with experiments on the pure methanol trimer leads to a structure for benzene(CH3OH)3 which incorporates a
hydrogen-bonded methanol trimer chain, confirming the earlier assignment based on its ultraviolet spectrum. The 3589 cm1 transition, due to the
hydrogen bond of the terminal methanol, is redshifted from the free monomer by 93 cm1, a value approaching that of the donor methanol in methanol dimer (107 cm1). The lower frequency transitions in the m=3 spectrum arise from the donoracceptor and donor OH stretches in the methanol trimer chain. The spectral characteristics change when m=4. The OH stretch transitions are all located in a region around 3320 cm1 and are significantly broadened compared to the smaller clusters. By comparison with ab initio calculations, the methanol tetramer structure in benzene(CH3OH)4 is deduced to be a cyclic methanol tetramer. The spectra for m=5 and 6 are slightly redshifted but similar to m=4 and point toward cyclic structures as well. ©1997 American Institute of Physics.
hydrogen bonding between benzene and methanol. The m=2 spectrum features two strong transitions at 3506 and 3605 cm1. The lower frequency peak is redshifted from the free monomer value by 175 cm1 and is assigned to the proton donor in the methanol dimer subcluster. The proton acceptor, which would be a free OH stretch in the absence of benzene, is redshifted by 76 cm1 due to a strengthened
hydrogen bond. In benzene(CH3OH)3, three sharp OH stretch transitions are observed at 3389, 3435, and 3589 cm1. The comparison of these absorptions with ab initio calculations and with experiments on the pure methanol trimer leads to a structure for benzene(CH3OH)3 which incorporates a
hydrogen-bonded methanol trimer chain, confirming the earlier assignment based on its ultraviolet spectrum. The 3589 cm1 transition, due to the
hydrogen bond of the terminal methanol, is redshifted from the free monomer by 93 cm1, a value approaching that of the donor methanol in methanol dimer (107 cm1). The lower frequency transitions in the m=3 spectrum arise from the donoracceptor and donor OH stretches in the methanol trimer chain. The spectral characteristics change when m=4. The OH stretch transitions are all located in a region around 3320 cm1 and are significantly broadened compared to the smaller clusters. By comparison with ab initio calculations, the methanol tetramer structure in benzene(CH3OH)4 is deduced to be a cyclic methanol tetramer. The spectra for m=5 and 6 are slightly redshifted but similar to m=4 and point toward cyclic structures as well. ©1997 American Institute of Physics.
| History: | Received 13 June 1996; accepted 7 November 1996 |
| Permalink: |
http://link.aip.org/link/?JCPSA6/106/2145/1 |
KEYWORDS and PACS
organic compounds,
molecular clusters,
ab initio calculations,
infrared spectra,
red shift,
hydrogen bonds
- 33.20.Ea
Molecular properties and interactions with photons Molecular spectra Infrared spectra - 36.40.Mr
Studies of special atoms, molecules, and their ions; clusters Atomic and molecular clusters Spectroscopy and geometrical structure of clusters - 33.70.Jg
Molecular properties and interactions with photons Intensities and shapes of molecular spectral lines and bands Line and band widths, shapes, and shifts - 33.15.Fm
Molecular properties and interactions with photons Properties of molecules and molecular ions Bond strengths, dissociation energies - YEAR: 1996-97
PUBLICATION DATA
0021-9606 (print)
1089-7690 (online)
There are no references.








